We present the results from almost-daily radio monitoring of supernova 1994I in M51, beginning one day after optical discovery. Using the Very Large Array (VLA) to monitor the supernova at 1.3, 2, 3.6, 6, and 20cm, we have obtained the most detailed radio light-curves yet of a type Ib/c supernova.
American Astronomical Society Meeting Abstracts
- Pub Date:
- December 1994